Testing the survival of microfossils in artificial martian sedimentary meteorites during entry into Earth's atmosphere: the STONE 6 experiment

Frédéric Foucher (1) , Francès Westall (1) , Franz Brandstätter (2) , René Demets (3) , John Parnell (4) , Charles S. Cockell (5) , Howell G.M. Edwards (6) , Jean-Michel Bény (7) , André Brack (1)

1 CBM - Centre de biophysique moléculaire
2 Naturhistorisches Museum Vienna
3 ESTEC - European Space Research and Technology Centre
4 School of Geosciences
5 PSSRI - Planetary and Space Sciences Research Institute [Milton Keynes]
6 Chemical and Forensic Sciences [Bradford]
7 ISTO - Institut des Sciences de la Terre d'Orléans

If life ever appeared on Mars, could we find traces of primitive life embedded in sedimentary meteorites? To answer this question, a 3.5 billion-year-old volcanic sediment containing microfossils was embedded in the heat shield of a space capsule in order to test survival of the rock and the microfossils during entry into the Earth's atmosphere (the STONE 6 experiment). The silicified volcanic sediment from the Kitty's Gap Chert (Pilbara, Australia) is considered to be an excellent analogue for Noachian-age volcanic sediments. The microfossils in the chert are also analogues for potential martian life. An additional goal was to investigate the survival of living microorganisms (Chroococcidiopsis) protected by a 2 cm thick layer of rock in order to test whether living endolithic organisms could survive atmospheric entry when protected by a rocky coating. Mineralogical alteration of the sediment due to shock heating was manifested by the formation of a fusion crust, cracks in the chert due to prograde and retrograde changes of α quartz to β quartz, increase in the size of the fluid inclusions, and dewatering of the hydromuscovite-replaced volcanic protoliths. The carbonaceous microfossils embedded in the chert matrix survived in the rock away from the fusion crust but there was an increase in the maturity index of the kerogen towards the crust. We conclude that this kind of sediment can survive atmospheric entry and, if it contains microfossils, they could also survive. The living microorganisms were, however, completely carbonised by flame leakage to the back of the sample and therefore non-viable. However, using an analytical model to estimate the temperature reached within the sample thickness, we conclude that, even without flame leakage, the living organisms probably need to be protected by at least 5 cm of rock in order to be shielded from the intense heat of entry.

Mots clés: Meteorites; Thermal histories; Astrobiology; Mineralogy; Mars

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Planétologie et astrophysique de la terre [astro-ph.EP]

Frédéric Foucher, Francès Westall, Franz Brandstätter, René Demets, John Parnell, et al.. Testing the survival of microfossils in artificial martian sedimentary meteorites during entry into Earth's atmosphere: the STONE 6 experiment. Icarus, 2010, 207 (2), pp.616-630. ⟨10.1016/j.icarus.2009.12.014⟩. ⟨insu-00444343⟩